Hydrogen Loss on Venus Driven by Photochemistry

Venus has experienced substantial H loss through hydrodynamic outflow in its early history, transforming from a warm and wet state to the current arid and scorching state. While Venus continues to lose H today, no consensus has been reached regarding the present dominant escape mechanisms. Recently,...

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書誌詳細

主要な著者:	Hao Gu, Jun Cui, Xiaoshu Wu, Xu Huang, Shiqi Wu, Wenlong Li, Jinjin Zhao, Haoyu Lu, Lei Li
フォーマット:	Artigo
言語:	Inglês
出版事項:	IOP Publishing 2025-01-01
シリーズ:	The Astrophysical Journal Letters
主題:	Venus Planetary atmospheres Atmospheric evolution Upper atmosphere Solar system terrestrial planets
オンライン･アクセス:	https://doi.org/10.3847/2041-8213/adec90
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